Semi-empirical models of the white-light flare on October 24, 1991     

C. Fang  J. C. Hénoux  Hu Ju  Xue Yin-Zhang  Gao Xiu-fa  Fu Qi-Jun 《Solar physics》1995,157(1-2):271-283

On October 24, 1991, a white-light flare was observed both from space and from the ground. A multi-waveband spectral analysis shows that the peak time of the continuum emission coincides well with that of a radio burst at 2840 MHz and with the hard X-ray emission. Three semi-empirical models, corresponding to the pre-flare condition and to the peak time of continuum emission both with and without non-thermal excitation and ionization of hydrogen by an electron beam, have been obtained. The results indicate that there is fast heating both in the chromosphere and the photosphere. Some evidence is given that this WLF is very likely a result of bombardment by an electron beam. By taking into account non-thermal effects, the chromospheric temperature of the semi-empirical model is significantly reduced.  相似文献   

Observations of the cosmic microwave background and galactic foregrounds at 12–17 GHz with the COSMOSOMAS experiment     

S. Fernández-Cerezo  C. M. Gutiérrez  R. Rebolo  R. A. Watson  R. J. Hoyland  S. R. Hildebrandt  J. A. Rubiño-Martín  J. F. Macías-Pérez  P. Sosa Molina 《Monthly notices of the Royal Astronomical Society》2006,370(1):15-24

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Groups of galaxies: relationship between environment and galaxy properties     

Héctor J. Martínez  Hernán Muriel 《Monthly notices of the Royal Astronomical Society》2006,370(2):1003-1007

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Use of the Geometric Elements in Numerical Simulations     

Stéfan Renner  Bruno Sicardy 《Celestial Mechanics and Dynamical Astronomy》2006,94(2):237-248

We derive the transformations to convert the state vector in cartesian coordinates into geometric orbital elements (and conversely the geometric elements into the state vector) for a test particle moving around an oblate planet. These transformations arise from the epicyclic theory and are accurate to second order in eccentricity and inclination. This paper is written to be directly used for computational purposes, such as the numerical study of ring dynamics.  相似文献   

Filaments within the Perseid meteoroid stream and their coincidence with the location of mean-motion resonances     

Ján Svoreň  Zuzana Kaňuchová  Marián Jakubík 《Icarus》2006,183(1):115-121

Positions of 17 filaments found inside the Perseid meteoroid stream by method of indices are compared with those of low-order mean-motion resonances with Jupiter and Saturn. By this comparing, the Jupiter and Saturn branches of the Perseid stream were identified. The existence of gaps in the distribution of the semi-major axes of the Perseids is confirmed using the more numerous material of a new version of the IAU Meteor Data Center Catalogue. Our integrations of the motion of particles in the Perseid stream lead to an extraordinary important fact. The found filaments are located in close proximity of strong resonances. They represent, with a high probability, increased numbers of particles gravitationally expelled from a resonant gap and (temporary) settled down in its close proximity.  相似文献   

Putative Meteoritic Craters in Río Cuarto (Central Argentina) Interpreted as Eolian Structures     

Cione  Alberto L.  Tonni  Eduardo P.  San Cristóbal  Jorge  Hernández  Pedro J.  Benítez  Adrián  Bordignon  Fernando  Perí  Jorge A. 《Earth, Moon, and Planets》2002,91(1):9-24

Ten oblong aligned depressions in the Río Cuarto area (provincia de Córdoba, Argentina) were supposed to be the result of very-low-angle Holocene meteoroid impacts. However, we consider that authors that studied the structures did not demonstrated their extraterrestrial origin. We suggest that an eolian origin for the structures of Río Cuarto is more likely. Actually, these landforms integrate large systems of similar deflation/accumulation geoforms aligned according to predominant winds during different periods.  相似文献   

Non-equilibrium beta processes in neutron stars: a relationship between the net reaction rate and the total emissivity of neutrinos     

Sergio Flores-Tulián  Andreas Reisenegger 《Monthly notices of the Royal Astronomical Society》2006,372(1):276-278

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Orbit Determination of Binary Asteroids     

Daniel Hestroffer  Frédéric Vachier  Benjamin Balat 《Earth, Moon, and Planets》2005,97(3-4):245-260

In addition to the detection of an asteroid moon or a binary asteroid, the knowledge of the satellite’s true orbit is of high importance to derive fundamental physical parameters of the binary system such as its mass and to shed light on its possible formation history and dynamical evolution (prograde/retrograde orbit, large/small eccentricity or inclination, etc.). A new methodology for preliminary orbit determination of binary asteroids – and visual binaries in general – is proposed. It is based on Thiele–Innes method combined with a ‘trial and error’ Monte-Carlo technique. This method provides the full set of solutions (bundle of orbits, with the 7 orbital elements) even for a reduced number of observations. The mass is a direct by-product of this orbit determination, from which one can next infer the bulk-density and porosity. In addition to the bundle of orbits, the method provides the marginal probability densities of the foreseen parameters. Such error analysis – since it avoids linear approximation – can be of importance for the prediction of the satellite’s position in the plane-of-sky during future stellar occultations or subsequent observations, but also for the analysis of the orbit’s secular evolution. After briefly describing the method, we present the algorithm and its application to some practical cases, with particular emphasis on asteroids binaries and applications on orbital evolution.  相似文献   

Near-infrared surface brightness fluctuations and optical colours of Magellanic star clusters     

R. A. González-Lópezlira  M. Y. Albarrán  M. Mouhcine  M. C. Liu †  G. Bruzual-A.  B. de Batz 《Monthly notices of the Royal Astronomical Society》2005,363(4):1279-1289

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Local And Global Diffusion Along Resonant Lines in Discrete Quasi-integrable Dynamical Systems     

Claude Froeschlé  Massimiliano Guzzo  Elena Lega 《Celestial Mechanics and Dynamical Astronomy》2005,92(1-3):243-255

We detect and measure diffusion along resonances in a quasi-integrable symplectic map for different values of the perturbation parameter. As in a previously studied Hamiltonian case (Lega et al., 2003) results agree with the prediction of the Nekhoroshev theorem. Moreover, for values of the perturbation parameter slightly below the critical value of the transition between Nekhoroshev and Chirikov regime we have also found a diffusion of some orbits along macroscopic portions of the phase space. Such a diffusion follows in a spectacular way the peculiar structure of resonant lines.  相似文献